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Open AccessJournal ArticleDOI

Spectrophotometric time series of SN 2011fe from the Nearby Supernova Factory

TLDR
In this paper, 32 epochs of optical (3300-9700 A) spectrophotometric observations of the nearby quintessential "normal" type Ia supernova (SN Ia) SN 2011fe in the galaxy M101, extending from -15 to +97 d with respect to B-band maximum, obtained by the Nearby Supernova Factory collaboration.
Abstract
We present 32 epochs of optical (3300-9700 A) spectrophotometric observations of the nearby quintessential "normal" type Ia supernova (SN Ia) SN 2011fe in the galaxy M101, extending from -15 to +97 d with respect to B-band maximum, obtained by the Nearby Supernova Factory collaboration. SN 2011fe is the closest (\mu = 29.04) and brightest (Bmax = 9.94 mag) SN Ia observed since the advent of modern large scale programs for the intensive periodic followup of supernovae. Both synthetic light curve measurements and spectral feature analysis attest to the normality of SN 2011fe. There is very little evidence for reddening in its host galaxy. The homogeneous calibration, intensive time sampling, and high signal-to-noise ratio of the data set make it unique. Thus it is ideal for studying the physics of SN Ia explosions in detail, and for furthering the use of SNe Ia as standardizable candles for cosmology. Several such applications are shown, from the creation of a bolometric light curve and measurement of the 56Ni mass, to the simulation of detection thresholds for unburned carbon, direct comparisons with other SNe Ia, and existing spectral templates.

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Journal ArticleDOI

Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

Marc Betoule, +72 more
TL;DR: In this article, the authors presented cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observations obtained by the SDSS-II and SNLS collaborations.
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An Open Catalog for Supernova Data

TL;DR: The Open Supernova Catalog (OSC) as discussed by the authors is a collection of observations and metadata for 36,000+ supernovae and related candidates, with its main interface designed to be a user-friendly, rapidly searchable table accessible on desktop and mobile devices.
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Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger.

TL;DR: In this article, the authors reported time-series spectroscopy of SSS17a from 11.75 hours until 8.5 days after the merger, and measured the photosphere cooling from 11, 000 − 900 + 3400 to 9300 − 300 + 300 kelvin and determined a photospheric velocity of roughly 30% of the speed of light.
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SOUSA: the Swift Optical/Ultraviolet Supernova Archive

TL;DR: The Swift Optical/Ultraviolet Supernova Archive (SOUSA) as discussed by the authors contains all of the supernova images and photometry from the UAV-UAV system, covering all major types and most subtypes.
References
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Journal ArticleDOI

Multi-epoch high-resolution spectroscopy of SN2011fe - Linking the progenitor to its environment

TL;DR: In this paper, high-resolution spectroscopy of SN2011fe on 12 epochs, from 8 to 86 days after the estimated date of explosion, targeting in particular at the time evolution of CaII and NaI.
Journal ArticleDOI

Type Ia Single Degenerate Survivors Must Be Overluminous

TL;DR: In the single-degenerate (SD) channel of a Type Ia supernovae (SN Ia) explosion, a main-sequence (MS) donor star survives the explosion but it is stripped of mass and shock heated.
Journal ArticleDOI

Multi-epoch Spectropolarimetry of SN 2011fe

TL;DR: In this article, multiple spectropolarimetric observations of the nearby Type Ia supernova SN 2011fe in M101 were obtained before, during, and after the time of maximum apparent visual brightness.
Posted Content

The supernova Ia 2011fe in M101, its tip of the red-giant branch (TRGB) distance, and the value of H_0

TL;DR: In this paper, the light curve parameters of the normal type Ia SN2011fe are derived from the rich archive of the AAVSO, and they are inserted into the Hubble line defined by 62 SNe Ia with 3000 < v < 20,000 km/s.
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